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Exact critical bubble free energy and the effectiveness of effective potential approximations

David E. Brahm*

Clarence L. Y. Lee

  • Carnegie Mellon, Pittsburgh, Pennsylvania 15213

  • California Institute of Technology, Pasadena, California 91125

  • *Electronic address: brahm@fermi.phys.cmu.edu
  • Electronic address: lee@theory3.caltech.edu

Phys. Rev. D 49, 4094 – Published 15 April, 1994

DOI: https://doi.org/10.1103/PhysRevD.49.4094

Abstract

To calculate the temperature at which a first-order cosmological phase transition occurs, one must calculate Fc(T), the free energy of a critical bubble configuration. Fc(T) is often approximated by the classical energy plus an integral over the bubble of the effective potential; one must choose a method for calculating the effective potential when V<0. We test different effective potential approximations at one loop. The agreement is best if one pulls a factor μ4T4 into the decay rate prefactor [where μ2=V(φf)], and takes the real part of the effective potential in the region V<0. We perform a similar analysis on the one-dimensional kink.

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